Core formation in dwarf haloes with self-interacting dark matter: no fine-tuning necessary
about
Galaxy formation with BECDM - I. Turbulence and relaxation of idealized haloes.The impact of baryonic physics on the structure of dark matter haloes: the view from the FIRE cosmological simulationsFrom cusps to cores: a stochastic modelMassive black holes from dissipative dark matterDensity profile of dark matter haloes and galaxies in the horizon–agn simulation: the impact of AGN feedback
P2860
Core formation in dwarf haloes with self-interacting dark matter: no fine-tuning necessary
description
im August 2015 veröffentlichter wissenschaftlicher Artikel
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wetenschappelijk artikel
@nl
наукова стаття, опублікована в серпні 2015
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name
Core formation in dwarf haloes ...... tter: no fine-tuning necessary
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Core formation in dwarf haloes ...... tter: no fine-tuning necessary
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type
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Core formation in dwarf haloes ...... tter: no fine-tuning necessary
@en
Core formation in dwarf haloes ...... tter: no fine-tuning necessary
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prefLabel
Core formation in dwarf haloes ...... tter: no fine-tuning necessary
@en
Core formation in dwarf haloes ...... tter: no fine-tuning necessary
@nl
P2093
P2860
P356
P1476
Core formation in dwarf haloes ...... tter: no fine-tuning necessary
@en
P2093
Annika H. G. Peter
James S. Bullock
Miguel Rocha
Oliver D. Elbert
P2860
P356
10.1093/MNRAS/STV1470
P407
P577
2015-08-12T00:00:00Z
P5875
P818
P819
2015MNRAS.453...29E